Add to ORKGThe chemical composition of the Sun provides the reference standard for a wide variety of astronomical, cosmochemical and geochemical studies. To better determine the solar composition, the Genesis spacecraft collected solar wind at the L1 point in space for 27 months from December 2001 to April 2004. Prior SIMS analyses of Genesis samples have found discrepant results for the Mg and Fe solar wind fluences from different collector materials (Burnett et al., 2007)
We present the elemental and isotopic composition of noble gases in the bulk solar wind collected by...
Abstract. Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ul...
Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high p...
The chemical composition of the Sun provides the reference standard for a wide variety of astronomic...
The chemical composition of the Sun provides the reference standard for a wide variety of astronomi...
The Genesis Discovery Mission returned samples of solar matter by exposing ultrapure materials to t...
We present elemental abundance data of C, N, O, Na, Mg, Al, Ca, and Cr in Genesis silicon targets. F...
NASA's Genesis mission was flown to capture samples of the solar wind and return them to the Earth f...
Genesis, a NASA sample return mission, collected solar wind (SW) in space for 2.5 years for precise...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
We present elemental abundance data of C, N, O, Na, Mg, Al, Ca, and Cr in Genesis silicon targets. F...
To meet the Genesis mission goal for improved solar elemental abundances, we need to address the iss...
The Genesis Discovery mission will return samples of solar matter for analysis of isotopic and eleme...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
Launched on 8 August 2001, the NASA Genesis mission is now collecting samples of the solar wind in v...
We present the elemental and isotopic composition of noble gases in the bulk solar wind collected by...
Abstract. Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ul...
Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high p...
The chemical composition of the Sun provides the reference standard for a wide variety of astronomic...
The chemical composition of the Sun provides the reference standard for a wide variety of astronomi...
The Genesis Discovery Mission returned samples of solar matter by exposing ultrapure materials to t...
We present elemental abundance data of C, N, O, Na, Mg, Al, Ca, and Cr in Genesis silicon targets. F...
NASA's Genesis mission was flown to capture samples of the solar wind and return them to the Earth f...
Genesis, a NASA sample return mission, collected solar wind (SW) in space for 2.5 years for precise...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
We present elemental abundance data of C, N, O, Na, Mg, Al, Ca, and Cr in Genesis silicon targets. F...
To meet the Genesis mission goal for improved solar elemental abundances, we need to address the iss...
The Genesis Discovery mission will return samples of solar matter for analysis of isotopic and eleme...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
Launched on 8 August 2001, the NASA Genesis mission is now collecting samples of the solar wind in v...
We present the elemental and isotopic composition of noble gases in the bulk solar wind collected by...
Abstract. Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ul...
Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high p...